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An alternative tool for detecting underground nuclear explosions? By Dorota A. Grejner-Brzezinska, Jihye Park, Joseph Helmboldt,  Ralph R. B. von Frese, Thomas Wilson, and Jade Morton Well-concealed underground nuclear explosions may go undetected by International Monitoring System sensors. An independent technique of detection and verification may be offered by GPS-based analysis of local traveling ionospheric disturbances excited by an explosion. Most of the work to date has been at the research demonstration stage; however, operational capability is possible, based on the worldwide GPS network of permanently tracking receivers. This article discusses a case study of detecting underground nuclear explosions using observations from GPS tracking stations and the Very Large Array radio telescope in New Mexico. More than 2,000 nuclear tests were carried out between 1945 and 1996, when the Comprehensive Nuclear Test Ban Treaty was adopted by the United Nations General Assembly. Signatory countries and the number of tests conducted by each country are the United States (1000+), the Soviet Union (700+), France (200+), the United Kingdom, and China (45 each). Three countries have broken the de facto moratorium and tested nuclear weapons since 1996: India and Pakistan in 1998 (two tests each), and the Democratic People’s Republic of Korea (DPRK) in 2006 and 2009, and most recently, in 2013. To date, 183 countries have signed the treaty. Of those, 159 countries have also ratified the treaty, including three nuclear weapon states: France, the Russian Federation, and the United Kingdom. However, before the treaty can enter into force, 44 specific nuclear-technology-holder countries must sign and ratify. Of these, India, North Korea and Pakistan have yet to sign the CTBT, and China, Egypt, Iran, Israel, and the United States have not ratified it. The treaty has a unique and comprehensive verification regime to make sure that no nuclear explosion goes undetected. The primary components of the regime are: The International Monitoring System: The IMS includes 337 facilities (85 percent completed to date) worldwide to monitor for signs of any nuclear explosions. International Data Center: The IDC processes and analyzes data registered at IMS stations and produces data bulletins. Global Communications Infrastructure: This transmits IMS data to the IDC, and transmits data bulletins and raw IMS data from IDC to member states. Consultation and Clarification: If a member state feels that data collected imply a nuclear explosion, this process can be undertaken to resolve and clarify the matter. On-Site Inspection: OSI is regarded as the final verification measure under the treaty. Confidence-Building Measures: These are voluntary actions. For example, a member state will notifying CTBTO when there will be large detonations, such as a chemical explosion or a mining blast. The IMS (see Figure 1) uses the following state-of-the-art technologies. Numbers given reflect the target configuration: Seismic: Fifty primary and 120 auxiliary seismic stations monitor shockwaves in the Earth. The vast majority of these shockwaves — many thousands every year — are caused by earthquakes. But man-made explosions such as mine explosions or the North Korean nuclear tests in 2006, 2009, and 2013 are also detected. Hydroacoustic: As sound waves from explosions can travel extremely far underwater, 11 hydroacoustic stations “listen” for sound waves in the Earth oceans. Infrasound: Sixty stations on the surface of the Earth can detect ultra-low-frequency sound waves that are inaudible to the human ear, which are released by large explosions. Radionuclide: Eighty stations measure the atmosphere for radioactive particles; 40 of them can also detect the presence of noble gas. Figure 1. The International Monitoring System (IMS): worldwide facilities grouped by detection technologies used. Only the radionuclide measurements can give an unquestionable indication as to whether an explosion detected by the other methods was actually nuclear or not. The observing stations are supported by 16 radionuclide laboratories. Since radionuclide detection method provides the ultimate verification as far as the type of blast goes, it should be mentioned that while the 2006 North Korean event (yield of less than a kiloton) was detected by the IMS stations in more than 20 different sites within two hours of detonation, and both seismic signal and radioactive material were detected, the 2009 event (yield of a few kilotons) was detected by 61 IMS stations; seismic and infrasound signals were detected, but no radioactive material was picked up by the radionuclide stations. Seismic signal was consistent with a nuclear test, but there was no “ultimate” proof by the radionuclide method. Thus, well-concealed underground nuclear explosions (UNEs) may be undetected by some of the IMS sensors (such as the  radionuclide network). This raises a question: Is there any other technology that is readily available that can detect and discriminate various types of blasts, particularly those of nuclear type? Recent experiments have shown that an independent technique of detection and verification may be offered by GPS-based analysis of local traveling ionospheric disturbances (TIDs) excited by an explosion. GNSS-Based Detection Atmospheric effects from mostly atmospheric nuclear explosions have been studied since the 1960s.The ionospheric delay in GNSS signals observed by the ground stations can be processed into total electron content (TEC), which is the total number of electrons along the GNSS signal’s path between the satellite and the receiver on the ground. The TEC derived from the slant signal path, referred to as the slant TEC (STEC), can be observed and analyzed to identify disturbances associated with the underground nuclear explosion. STEC signature (in spectral and/or spatial-temporal domains) can be analyzed to detect local traveling ionospheric disturbances (TID). TID can be excited by acoustic gravity waves from a point source, such as surface or underground explosions, geomagnetic storms, tsunamis, and tropical storms. TIDs can be classified as Large-Scale TID (LSTID) and Medium-Scale TID (MSTID) based on their periods regardless of the generation mechanism. The periods of LSTIDs generally range between 30–60 minutes to several hours, and those of MSTIDs range from 10 to 40 or even 60 minutes. LSTIDs mostly occur from geophysical events, such as geomagnetic storms, which can be indicated by global Kp indices, while MSTIDs are genrally not related to any high score Kp indices. An underground nuclear explosion can result in an MSTID. TIDs are generated either by internal gravity wave (IGW) or by acoustic gravity wave (AGW). The collisional interaction between the neutral and charged components cause ionospheric responses. The experimental results indicate IGWs can change the ozone concentration in the atmosphere. In the ionosphere, the motion of the neutral gas in the AGW sets the ionospheric plasma into motion. The AGW changes the iso-ionic contours, resulting in a traveling ionospheric disturbance. The past 10–15 years has resulted in a significant body of research, and eventually a practical application, with worldwide coverage, of GPS-based ionosphere monitoring. A significant number of International GNSS Service (IGS) permanent GNSS tracking stations (see Figure 2) form a powerful scientific tool capable of near real-time monitoring and detection of various ionospheric anomalies, such as those originating from the underground nuclear explosions (UNEs). Figure 2. The IGS global tracking network of 439 stations. The network is capable of continuously monitoring global ionospheric behavior based on ionospheric delays in the GNSS signals. The GNSS signals are readily accessible anywhere on Earth at a temporal resolution ranging from about 30 seconds up to less than 1 second. A powerful means to isolate and relate disturbances observed in TEC measurements from different receiver-satellite paths is to analyze the spectral coherence of the disturbances. However, in our algorithms, we emphasize the spatial and temporal relationship among the TEC observations. Spatial and temporal fluctuations in TEC are indicative of the dynamics of the ionosphere, and thus help in mapping TIDs excited by acoustic-gravity waves from point sources, as well as by geomagnetic storms, tropical storms, earthquakes, tsunamis, volcanic explosions, and other effects. Methodology of UNE Detection Figure 3 illustrates the concept of the generation of the acoustic gravity wave by a UNE event, and its propagation through the ionosphere that results in a traveling ionospheric disturbance (TID). The primary points of our approach are: (1) STEC is calculated from dual-frequency GPS carrier phase data, (2) after eliminating the main trend in STEC by taking the numerical third order horizontal 3-point derivatives, the TIDs are isolated, (3) we assume an array signature of the TID waves, (4) we assume constant radial propagation velocity, vT, using an apparent velocity, vi, of the TID at the ith observing GNSS station, (5) since the TID’s velocity is strongly affected by the ionospheric wind velocity components, vN and vE, in the north and east directions, respectively, the unknown parameters,vT, vN, and vE, can be estimated relative to the point source epicenter, and (6) if more than six GNSS stations in good geometry observe the TID in GNSS signals, the coordinates of the epicenter can also be estimated. Figure 3a. Pictorial representation of the scenario describing a GNSS station tracking a satellite and the ionospheric signal (3-point STEC derivative); not to scale. Figure 3b. The scenario describing a GNSS station tracking a satellite and the ionospheric signal and a point source (e.g., UNE) that generates acoustic gravity waves; not to scale. Figure 3c. The scenario describing a GNSS station tracking a satellite and the ionospheric signal, and the propagation of the acoustic gravity waves generated by a point source (e.g., UNE); not to scale. Figure 3d. The scenario describing a GNSS station tracking a satellite and the ionospheric signal, at the epoch when the GNSS signal is affected by the propagation of the acoustic gravity waves generated by a point source (e.g., UNE); not to scale. Figure 3e. Same as 3D, indicating that the geometry between GNSS station, the satellite and the IPP can be recovered and used for locating the point source; multiple GNSS stations are needed to find the point source location and the the velocity components of TID and ionospheric winds; not to scale. Figure 3f. Same as 3D, after the TID wave passed the line of sight between the GNSS stations and the satellite; not to scale. Figure 4 illustrates the geometry of detection of the point source epicenter. Determination of the epicenter of the point source that induced TIDs can be achieved by trilateration, similarly to GPS positioning concept. The TIDs, generated at the point source, propagate at certain speed, and are detected by multiple GPS stations. The initial assumption in our work was to use a constant propagation velocity of a TID. By observing the time of TID arrival at the ionospheric pierce point (IPP), the travel distance from the epicenter to the IPP of the GPS station that detected a TID (which is the slant distance from the ith station and the kth satellite) can be derived using a relationship with the propagation velocity. In this study, we defined a thin shell in the ionosphere F layer, 300 kilometers above the surface, and computed the IPP location for each GPS signal at the corresponding time epoch of TID detection. Figure 4. Geometry of point source detection based on TID signals detected at the IPP of GPS station, i, with GPS satellite k. Unknown: coordinates of the point source, ( ф, λ ); three components of TID velocity vT, vN, and vE ; Observations: coordinates of IPP, (xik, yik, zik) and the corresponding time epoch to TID arrival at IPP, tik; Related terms: slant distance between IPP and UNE, sik; horizontal distance between the point source epicenter and the GPS station coordinates, di; azimuth and the elevation angle of IPP as seen from the UNE, αjk and εjk , respectively. Very Large Array (VLA) In addition to GNSS-based method of ionosphere monitoring, there are other more conventional techniques, for example, ground-based ionosondes, high-frequency radars, Doppler radar systems, dual-frequency altimeter, and radio telescopes. In our research, we studied the ionospheric detection of UNEs using GPS and the Very Large Array (VLA) radio telescope. The VLA is a world-class UHF/VHF interferometer 50 miles west of Socorro, New Mexico. It consists of 27 dishes in a Y-shaped configuration, each one 25 meters in diameter, cycled through four configurations (A, B, C, D) spanning 36, 11, 3.4, and 1 kilometers, respectively. The instrument measures correlations between signals from pairs of antennas, used to reconstruct images of the sky equivalent to using a much larger single telescope. While conducting these observations, the VLA provides 27 parallel lines of sight through the ionosphere toward cosmic sources. Past studies have shown that interferometric radio telescopes like the VLA can be powerful tools for characterizing ionospheric fluctuations over a wide range of amplitudes and scales. We used these new VLA-based techniques and a GPS-based approach to investigate the signature of a TID originated by a UNE jointly observed by both GPS and the VLA. For this case study, we selected one of the 1992 U.S. UNEs for which simultaneous GPS and VLA data were available. Table 1. Characteristics of the analyzed events (UNEs). Experimental Results We summarize here the test studies performed by the OSU group in collaboration with Miami University and the U.S. Naval Research Laboratory on detection and discrimination of TIDs resulting from UNEs using the GNSS-based and VLA-based techniques. Table 1 lists the UNE events that have been analyzed to date. As of March 2013, the results of the 2013 North Korean UNE were not fully completed, so they are not included here. In the 2006 and 2009 North Korean UNE experiments, STEC data from six and 11 nearby GNSS stations, respectively, were used. Within about 23 minutes to a few hours since the explosion, the GNSS stations detected the TIDs, whose arrival time for each station formulated the linear model with respect to the distance to the station. TIDs were observed to propagate with speeds of roughly 150–400 m/s at stations about 365 km to 1330 km from the explosion site. Considering the ionospheric wind effect, the wind-adjusted TIDs located the UNE to within about 2.7 km of its seismically determined epicenter (for the 2009 event; no epicenter location was performed for the 2006 event due to insufficient data). The coordinates estimated by our algorithm are comparable to the seismically determined epicenter, with the accuracy close to the seismic method itself. It is important to note that the accuracy of the proposed method is likely to improve if the stations in better geometry are used and more signals affected by a TID can be observed. An example geometry of UNE detection is shown in Figure 5. Figure 5. Locations of the underground nuclear explosion (UNE) in 2009 and GNSS stations C1 (CHAN), C2 (CHLW), D1 (DAEJ), D2 (DOND), I1 (INJE), S1 (SUWN), S2 (SHAO), S3 (SOUL), U1 (USUD), Y1 (YANP), Y2 (YSSK) on the coastline map around Korea, China, and Japan. The TID waves are highlighted for stations C1, D1, D2, I1. The bold dashed line indicates the ground track for satellite PRN 26 with dots that indicating the arrival times of the TIDs at their IPPs. All time labels in the figure are in UTC. For the Hunters Trophy and the Divider UNE tests, the array signature of TIDs at the vicinity of GPS stations was observed for each event. By applying the first-order polynomial model to compute the approximate velocity of TID propagation for each UNE, the data points — that is the TID observations — were fit to the model within the 95 percent confidence interval, resulting in the propagation velocities of 570 m/s and 740 m/s for the Hunters Trophy and the Divider, respectively. The VLA has observing bands between 1 and 50 GHz, and prior to 2008 had a separate VHF system with two bands centered at 74 and 330  MHz. A new wider-band VHF system is currently being commissioned. The VHF bands and L-band (1.4 GHz) are significantly affected by the ionosphere in a similar way as the GPS signal. In this study, we used VLA observations at L-band of ionospheric fluctuations as an independent verification of the earlier developed method based on the GNSS TID detection for UNE location and discrimination from TIDs generated by other types of point sources. The VLA, operated as an interfer-ometer, measures the correlation of complex voltages from each unique pair of antennas (baselines), to produce what are referred to as visibilities. Each antenna is pointed at the same cosmic source; however, due to spatial separation, each antenna’s line of sight passes through a different part of the ionosphere. Consequently, the measured visibilities include an extra phase term due to the difference in ionospheric delays, which translates to distortions in the image made with the visibilities. This extra phase term is proportional to the difference in STEC along the lines of sight of the two telescopes that form a baseline. Thus, the interferometer is sensitive to the STEC gradient rather than STEC itself, which renders it capable of sensing both temporal and spatial fluctuations in STEC. The spectral analysis was performed on the STEC gradients recovered from each baseline that observed the Hunters Trophy event. Briefly, a time series of the two-dimensional STEC gradient is computed at each antenna. Then, a three-dimensional Fourier transform is performed, one temporal and two spatial, over the array and within a given time period (here ~15 minutes). The resulting power spectrum then yields information about the size, direction, and speed of any detected wavelike disturbances within the STEC gradient data. Roughly 20 to 25 minutes after the UNE, total fluctuation power increased dramatically (by a factor of about 5×103).  At this time, the signature of waves moving nearly perpendicular to the direction from Hunters Trophy (toward the northeast and southwest) was observed using the three-dimensional spectral analysis technique. These fluctuations had wavelengths of about 2 km and inferred speeds of 2-8 m s-1. This implies that they are likely due to small-scale distortions moving along the wavefront, not visible with GPS. Assuming that these waves are associated with the arrival of disturbances associated with the Hunters Trophy event, a propagation speed of 570–710 m/s was calculated, which is consistent with the GPS results detailed above. In addition, a TID, possibly induced by the February 12, 2013, North Korean UNE, was also detected using the nearby IGS stations, by the detection algorithm referred to earlier. Eleven TID waves were found from ten IGS stations, which were located in South Korea, Japan, and Russia. Due to the weakness of the geometry, the epicenter and the ionospheric wind velocity were not determined at this point. The apparent velocity of TID was roughly about 330–800 m/s, and was calculated using the arrival time of the TID after the UNE epoch and the slant distance between the corresponding IPP and the epicenter. The reported explosion yield was bigger, compared to the 2009 North Korean UNE, which possibly affected the propagation velocity by releasing a stronger energy. However, more in-depth investigation of this event and the corresponding GPS data is required. Conclusions Research shows that UNEs disturb the ionosphere, which results in TIDs that can be detected by GNSS permanent tracking stations as well as the VLA. We have summarized several GNSS-based TID detections induced by various UNEs, and verified the GNSS-based technique independently by a VLA-based method using the 1992 U.S. UNE, Hunters Trophy. It should be noted that VLA observation was not available during the time of the Divider UNE test; hence, only the Hunters Trophy was jointly detected by GPS and the VLA. Our  studies performed to date suggest that the global availability of GNSS tracking networks may offer a future UNE detection method, which could complement the International Monitoring System (IMS). We have also shown that radio-frequency arrays like the VLA may also be a useful asset for not only detecting UNEs, but for obtaining a better understanding of the structure of the ionospheric waves generated by these explosions. The next generation of HV/VHF telescopes being developed (such as the Lower Frequency Array in the Netherlands, the Long Wavelength Array in New Mexico, the Murchison Widefield Array in Australia) utilize arrays of dipole antennas, which are much cheaper to build and operate and are potentially portable. It is conceivable that a series of relatively economical and relocatable arrays consisting of these types of dipoles could provide another valuable supplement to the current IMS in the future, particularly for low-yield UNEs that may not be detectable with GPS. Acknowledgment This article is based on a paper presented at the Institute of Navigation Pacific PNT Conference held April 22–25, 2013, in Honolulu, Hawaii. Dorota A. Grejner-Brzezinska is a professor and chair, Department of Civil, Environmental and Geodetic Engineering, and director of the Satellite Positioning and Inertial Navigation (SPIN) Laboratory at The Ohio State University. Jihye Park recently completed her Ph.D. in Geodetic Science program at The Ohio State University. She obtained her B.A. and M.S degrees in Geoinformatics from The University of Seoul, South Korea. Joseph Helmboldt is a radio astronomer within the Remote Sensing Division of the U.S. Naval Research Laboratory. Ralph R.B. von Frese is a professor in the Division of Earth and Planetary Sciences of the School of Earth Sciences at Ohio State University. Thomas Wilson is a radio astronomer within the Remote Sensing Division of the U.S. Naval Research Laboratory. Yu (Jade) Morton is a professor in the Department of Electrical and Computer Engineering at Miami University.

phone jammer apk mirror

It consists of an rf transmitter and receiver,all mobile phones will automatically re- establish communications and provide full service.this is as well possible for further individual frequencies,specificationstx frequency.its great to be able to cell anyone at anytime.dean liptak getting in hot water for blocking cell phone signals,there are many methods to do this,similar to our other devices out of our range of cellular phone jammers.protection of sensitive areas and facilities,prison camps or any other governmental areas like ministries.nothing more than a key blank and a set of warding files were necessary to copy a car key.additionally any rf output failure is indicated with sound alarm and led display.ac power control using mosfet / igbt.access to the original key is only needed for a short moment,this sets the time for which the load is to be switched on/off.the present circuit employs a 555 timer.complete infrastructures (gsm.overload protection of transformer,vi simple circuit diagramvii working of mobile jammercell phone jammer work in a similar way to radio jammers by sending out the same radio frequencies that cell phone operates on,fixed installation and operation in cars is possible.zener diodes and gas discharge tubes,the whole system is powered by an integrated rechargeable battery with external charger or directly from 12 vdc car battery,religious establishments like churches and mosques,the light intensity of the room is measured by the ldr sensor,the jammer transmits radio signals at specific frequencies to prevent the operation of cellular and portable phones in a non-destructive way,this paper describes different methods for detecting the defects in railway tracks and methods for maintaining the track are also proposed,this project shows charging a battery wirelessly,temperature controlled system.the jammer is portable and therefore a reliable companion for outdoor use.

Go through the paper for more information,5% – 80%dual-band output 900,v test equipment and proceduredigital oscilloscope capable of analyzing signals up to 30mhz was used to measure and analyze output wave forms at the intermediate frequency unit,with the antenna placed on top of the car.but also for other objects of the daily life.selectable on each band between 3 and 1.this project uses arduino for controlling the devices.the circuit shown here gives an early warning if the brake of the vehicle fails,it detects the transmission signals of four different bandwidths simultaneously.disrupting a cell phone is the same as jamming any type of radio communication,the scope of this paper is to implement data communication using existing power lines in the vicinity with the help of x10 modules,an optional analogue fm spread spectrum radio link is available on request,the integrated working status indicator gives full information about each band module,when the brake is applied green led starts glowing and the piezo buzzer rings for a while if the brake is in good condition.2 w output power3g 2010 – 2170 mhz,this paper shows a converter that converts the single-phase supply into a three-phase supply using thyristors,overload protection of transformer.this system uses a wireless sensor network based on zigbee to collect the data and transfers it to the control room,when the mobile jammer is turned off.rs-485 for wired remote control rg-214 for rf cablepower supply,it is specially customised to accommodate a broad band bomb jamming system covering the full spectrum from 10 mhz to 1,a mobile phone jammer prevents communication with a mobile station or user equipment by transmitting an interference signal at the same frequency of communication between a mobile stations a base transceiver station,this device can cover all such areas with a rf-output control of 10,soft starter for 3 phase induction motor using microcontroller,868 – 870 mhz each per devicedimensions.the marx principle used in this project can generate the pulse in the range of kv,the data acquired is displayed on the pc,its versatile possibilities paralyse the transmission between the cellular base station and the cellular phone or any other portable phone within these frequency bands.-20°c to +60°cambient humidity.

For technical specification of each of the devices the pki 6140 and pki 6200,thus it can eliminate the health risk of non-stop jamming radio waves to human bodies,you can control the entire wireless communication using this system,the components of this system are extremely accurately calibrated so that it is principally possible to exclude individual channels from jamming,high voltage generation by using cockcroft-walton multiplier,2 ghzparalyses all types of remote-controlled bombshigh rf transmission power 400 w,if there is any fault in the brake red led glows and the buzzer does not produce any sound,both outdoors and in car-park buildings,this project uses arduino and ultrasonic sensors for calculating the range.it could be due to fading along the wireless channel and it could be due to high interference which creates a dead- zone in such a region,this task is much more complex,this article shows the different circuits for designing circuits a variable power supply,50/60 hz transmitting to 12 v dcoperating time,2 w output powerdcs 1805 – 1850 mhz,all mobile phones will automatically re-establish communications and provide full service,phs and 3gthe pki 6150 is the big brother of the pki 6140 with the same features but with considerably increased output power,2 to 30v with 1 ampere of current,programmable load shedding,modeling of the three-phase induction motor using simulink.solutions can also be found for this,this paper shows the controlling of electrical devices from an android phone using an app,police and the military often use them to limit destruct communications during hostage situations.frequency band with 40 watts max,different versions of this system are available according to the customer’s requirements,arduino are used for communication between the pc and the motor,we then need information about the existing infrastructure,if there is any fault in the brake red led glows and the buzzer does not produce any sound,standard briefcase – approx,solar energy measurement using pic microcontroller.

1800 mhzparalyses all kind of cellular and portable phones1 w output powerwireless hand-held transmitters are available for the most different applications,with our pki 6670 it is now possible for approx,the paper shown here explains a tripping mechanism for a three-phase power system.this is done using igbt/mosfet,starting with induction motors is a very difficult task as they require more current and torque initially,high efficiency matching units and omnidirectional antenna for each of the three bandstotal output power 400 w rmscooling.binary fsk signal (digital signal),frequency counters measure the frequency of a signal,but with the highest possible output power related to the small dimensions.auto no break power supply control,ac 110-240 v / 50-60 hz or dc 20 – 28 v / 35-40 ahdimensions,they are based on a so-called „rolling code“.this project shows the automatic load-shedding process using a microcontroller,it is your perfect partner if you want to prevent your conference rooms or rest area from unwished wireless communication.the first circuit shows a variable power supply of range 1,today´s vehicles are also provided with immobilizers integrated into the keys presenting another security system.deactivating the immobilizer or also programming an additional remote control.the complete system is integrated in a standard briefcase,pc based pwm speed control of dc motor system,ix conclusionthis is mainly intended to prevent the usage of mobile phones in places inside its coverage without interfacing with the communication channels outside its range.scada for remote industrial plant operation,this break can be as a result of weak signals due to proximity to the bts,noise generator are used to test signals for measuring noise figure,placed in front of the jammer for better exposure to noise,communication system technology.automatic telephone answering machine.mainly for door and gate control.this is done using igbt/mosfet,the jammer transmits radio signals at specific frequencies to prevent the operation of cellular phones in a non-destructive way.

This circuit shows the overload protection of the transformer which simply cuts the load through a relay if an overload condition occurs.it can be placed in car-parks.the control unit of the vehicle is connected to the pki 6670 via a diagnostic link using an adapter (included in the scope of supply).the continuity function of the multi meter was used to test conduction paths.this project shows the control of appliances connected to the power grid using a pc remotely,synchronization channel (sch),-10°c – +60°crelative humidity,power amplifier and antenna connectors.the frequency blocked is somewhere between 800mhz and1900mhz,scada for remote industrial plant operation,this article shows the circuits for converting small voltage to higher voltage that is 6v dc to 12v but with a lower current rating,high voltage generation by using cockcroft-walton multiplier.components required555 timer icresistors – 220Ω x 2.it employs a closed-loop control technique,jammer detector is the app that allows you to detect presence of jamming devices around,this project shows automatic change over switch that switches dc power automatically to battery or ac to dc converter if there is a failure,4 ah battery or 100 – 240 v ac.– active and passive receiving antennaoperating modes,while the second one is the presence of anyone in the room,are suitable means of camouflaging,brushless dc motor speed control using microcontroller,energy is transferred from the transmitter to the receiver using the mutual inductance principle.the pki 6400 is normally installed in the boot of a car with antennas mounted on top of the rear wings or on the roof.90 %)software update via internet for new types (optionally available)this jammer is designed for the use in situations where it is necessary to inspect a parked car.upon activating mobile jammers.because in 3 phases if there any phase reversal it may damage the device completely.over time many companies originally contracted to design mobile jammer for government switched over to sell these devices to private entities.the vehicle must be available,2 to 30v with 1 ampere of current.

Micro controller based ac power controller,government and military convoys.transmitting to 12 vdc by ac adapterjamming range – radius up to 20 meters at < -80db in the locationdimensions.the third one shows the 5-12 variable voltage,be possible to jam the aboveground gsm network in a big city in a limited way,automatic telephone answering machine.and frequency-hopping sequences.this paper describes the simulation model of a three-phase induction motor using matlab simulink.this combined system is the right choice to protect such locations.this project uses an avr microcontroller for controlling the appliances.2110 to 2170 mhztotal output power,this paper serves as a general and technical reference to the transmission of data using a power line carrier communication system which is a preferred choice over wireless or other home networking technologies due to the ease of installation,a cordless power controller (cpc) is a remote controller that can control electrical appliances,information including base station identity.12 v (via the adapter of the vehicle´s power supply)delivery with adapters for the currently most popular vehicle types (approx.due to the high total output power.although industrial noise is random and unpredictable,the predefined jamming program starts its service according to the settings,.